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Valley formation by groundwater seepage, pressurized groundwater outbursts and crater-lake overflow in flume experiments with implications for Mars

Marra, Wouter A.; Braat, Lisanne; Baar, Anne W.; Kleinhans, Maarten G.

Authors

Wouter A. Marra

Lisanne Braat

Anne W. Baar

Maarten G. Kleinhans



Abstract

Remains of fluvial valleys on Mars reveal the former presence of water on the surface. However, the source of water and the hydrological setting is not always clear, especially in types of valleys that are rare on Earth and where we have limited knowledge of the processes involved. We investigated three hydrological scenarios for valley formation on Mars: hydrostatic groundwater seepage, release of pressurized groundwater and crater-lake overflow. Using physical modeling in laboratory experiments and numerical hydrological modeling we quantitatively studied the morphological development and processes involved in channel formation that result from these different sources of water in unconsolidated sediment. Our results show that valleys emerging from seeping groundwater by headward erosion form relatively slowly as fluvial transport takes place in a channel much smaller than the valley. Pressurized groundwater release forms a characteristic source area at the channel head by fluidization processes. This head consist of a pit in case of superlithostatic pressure and may feature small radial channels and collapse features. Valleys emerging from a crater-lake overflow event develop quickly in a run-away process of rim erosion and discharge increase. The valley head at the crater outflow point has a converging fan shape, and the rapid incision of the rim leaves terraces and collapse features. Morphological elements observed in the experiments can help in identifying the formative processes on Mars, when considerations of experimental scaling and lithological characteristics of the martian surface are taken into account. These morphological features might reveal the associated hydrological settings and formative timescales of a valley. An estimate of formative timescale from sediment transport is best based on the final channel dimensions for groundwater seepage valleys and on the valley dimensions for pressurized groundwater release and crater-lake overflow valleys. Our experiments show that different sources of water form valleys of similar size in quite different timescales.

Citation

Marra, W. A., Braat, L., Baar, A. W., & Kleinhans, M. G. (2014). Valley formation by groundwater seepage, pressurized groundwater outbursts and crater-lake overflow in flume experiments with implications for Mars. Icarus, 232, 97-117. https://doi.org/10.1016/j.icarus.2013.12.026

Journal Article Type Article
Acceptance Date Dec 26, 2013
Online Publication Date Jan 9, 2014
Publication Date 2014-04
Deposit Date Dec 6, 2019
Journal Icarus
Print ISSN 0019-1035
Publisher Elsevier
Peer Reviewed Peer Reviewed
Volume 232
Pages 97-117
DOI https://doi.org/10.1016/j.icarus.2013.12.026
Keywords Mars; Mars, surface; Geological processes; Experimental techniques
Public URL https://hull-repository.worktribe.com/output/2851459
Publisher URL https://www.sciencedirect.com/science/article/pii/S0019103514000086?via%3Dihub#!
Related Public URLs https://www.narcis.nl/publication/RecordID/oai%3Adspace.library.uu.nl%3A1874%2F307229/uquery/Valley%20formation%20by%20groundwater%20seepage/id/1/Language/en
Additional Information This article is maintained by: Elsevier; Article Title: Valley formation by groundwater seepage, pressurized groundwater outbursts and crater-lake overflow in flume experiments with implications for Mars; Journal Title: Icarus; CrossRef DOI link to publisher maintained version: https://doi.org/10.1016/j.icarus.2013.12.026; Content Type: article; Copyright: Copyright © 2014 Elsevier Inc. All rights reserved.